Zobrazeno 1 - 10
of 26
pro vyhledávání: '"F. T. Haddock"'
Autor:
William H. Potter, Joseph Fainberg, R. J. Fitzenreiter, Hector Alvarez, Richard R. Weber, F. T. Haddock
Publikováno v:
Solar Physics. 52:477-484
New observations of the out-of-the ecliptic trajectories of type III solar radio bursts have been obtained from simultaneous direction finding measurements on two independent satellite experiments, IMP-6 with spin plane in the ecliptic, and RAE-2 wit
Autor:
F. T. Haddock, Hector Alvarez
Publikováno v:
Solar Physics. 30:175-182
Type III bursts were observed between 3.5 MHz and 50 kHz by the University of Michigan radio astronomy experiment aboard the OGO-5 satellite.
Autor:
F. T. Haddock, Hector Alvarez
Publikováno v:
Solar Physics. 29:197-209
The analysis of type III bursts observed from the OGO-5 satellite between 3.5 MHz and 50 kHz (λ6 km) gives an empirical expression for the frequency drift rate as a function of frequency that is valid from 75 kHz to 550 MHz. Using this expression an
Autor:
M. R. Kundu, F. T. Haddock
Publikováno v:
Nature. 186:610-613
Results are reported from a statistical study of the nature of centimeter-wave as well as meter-wave radio outbursts associated with polar cap absorption events. General conclusions are drawn regarding the prediction of the proton events. (C.H.)
Autor:
F. T. Haddock
Publikováno v:
Symposium - International Astronomical Union. 9:188-193
The sun has been observed daily at the University of Michigan during the last year with three sweep-frequency receivers covering the 100 to 580 Mc/s band three times a second. The output is displayed as an intensity-modulated line on a precision cath
Publikováno v:
Solar Physics. 31:493-500
We have grouped observed type III solar bursts according to the discrete frequencies of observation in the kilometric wavelength range. For each group we have obtained the bursts' frequency of occurrence as a function of the heliographic longitude of
Autor:
F. T. Haddock
Publikováno v:
Symposium - International Astronomical Union. 4:192-196
This talk is based largely upon the centimetre-wave observations of hydrogen emission nebulae made with the Naval Research Laboratory 50-ft. paraboloidal reflector at 3·15 cm. [1], at 9·4 cm. [2], and at 21 cm. [3]. After the detection of the first
Publikováno v:
Solar Physics. 26:468-473
Type III radio bursts observed at kilometric wavelengths (less than or about equal to 0.35 MHz) by the Ogo-5 spacecraft are compared with greater than 45 keV solar electron events observed near 1 AU by the IMP-5 and Explorer 35 spacecraft for the per
Autor:
F. T. Haddock, D. Walsh
Publikováno v:
Symposium - International Astronomical Union. 23:335-343
A critical review is given of the theory and experimental observations of antenna impedance behaviour in a plasma, as related to radio astronomy. The emphasis is on electrically small antennas. Three simplified cases of plasma are considered, namely,
Autor:
F. T. Haddock
Publikováno v:
Proceedings of the IRE. 46:3-12
A general description of the nature of radio astronomy, its differences from optical astronomy, a review of the earliest beginnings of galactic and solar radio astronomy, and a listing of other important observational discoveries is given. A nearly c